Mars orbiter captures striking images of ‘chaos and craters’ carved by ancient floods

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Stunning new images from Europe’s Mars Express orbiter reveal a rugged Martian landscape carved by catastrophic floods that once tore across the Red Planet billions of years ago.

The dramatic new view, released by the European Space Agency (ESA) on May 13, spotlights Shalbatana Vallis, a sprawling Martian channel system near the planet’s equator that stretches roughly 800 miles (1,300 kilometers, or about the length of Italy. The image was taken by Mars Express’ High Resolution Stereo Camera (HRSC), highlighting what planetary scientists call “chaotic terrain,” according to a statement from the space agency.

“This kind of terrain is common on Mars, and has been captured before by Mars Express,” ESA officials said in the statement.

Researchers believe huge quantities of groundwater likely burst onto the surface in a series of catastrophic floods that surged downhill and rapidly carved the waterworn valleys visible today. The main channel seen in the images measures about 6 miles (10 kilometers) wide and plunges roughly 1,640 feet (500 meters) deep.

Looking down on a patch of Mars's surface, with a winding canyon carving from the left to the right of the frame. On the left, the canyon widens and is filled with lumpy, knobbly terrain. On the right, the canyon is more straight and streamlined. Surrounding the canyon is more lumpy terrain, but on top of a smoother surface

A new image from ESA’s Mars Express shows part of Shalbatana Vallis, a large channel in Mars’s equatorial region. (Image credit: ESA/DLR/FU Berlin)

The recent images also reveal layers of Mars’ complex geological past across the region, suggesting Shalbatana Vallis may once have been even deeper before gradually filling in with sediments, ash and other material over time. Dark blue-black deposits scattered through the valley are thought to be volcanic ash redistributed by Martian winds, while impact craters, wrinkle ridges and isolated mesas point to repeated cycles of catastrophic flooding, lava flows and erosion spanning billions of years.

A dark orange patch of Mars, with a large, winding channel running from the bottom left to the right of the frame. The rest of the landscape is scattered with circular craters and uneven bumps, but is mostly smooth. A small scale bar at the bottom right indicates that north is to the left, and that a line approximately one tenth of the image width is 20 km long.

Mars Express imagery of a part of a small patch of chaotic terrain within Shalbatana Vallis, a large channel near Mars’s equator. (Image credit: ESA/DLR/FU Berlin)

Scientists are especially interested in regions like Shalbatana Vallis because they preserve evidence that Mars was once far warmer and wetter than it is today. The channel empties toward Chryse Planitia, one of the lowest regions on Mars, where some researchers have proposed an ancient ocean may once have existed, according to the statement.

Launched in 2003, Mars Express remains one of the longest-running missions still operating at Mars, with its HRSC mapping the Red Planet in color and 3D for more than two decades. Over the course of its mission, the spacecraft has played a major role in uncovering evidence of Mars’ watery past, mapping minerals formed in water, studying buried ice deposits and even contributing to controversial findings suggesting possible liquid water beneath the planet’s southern polar ice cap.

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